The IBEX-Lo Sensor

By S. Fuselier, P. Bochsler, D. Chornay, G. Clark, Geoff Crew, G. Dunn, S. Ellis, T. Friedmann, H. Funsten, A. Ghielmetti and 38 more. 2009

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INTERSTELLAR GAS FLOW PARAMETERS DERIVED FROM INTERSTELLAR BOUNDARY EXPLORER-Lo OBSERVATIONS IN 2009 AND 2010: ANALYTICAL ANALYSIS (2012, methodology): “IBEX-Lo is described in detail by Fuselier et al. (2009).”
NEUTRAL INTERSTELLAR HELIUM PARAMETERS BASED ON IBEX-Lo OBSERVATIONS AND TEST PARTICLE CALCULATIONS (2012, methodology): “The field of view (FOV) of IBEX-Lo was defined in the simulation program according to the FOV specification for IBEXLo (Fuselier et al. 2009), and in a separate study (Hłond et al. 2012), it was verified that the pointing of IBEX-Lo indeed agrees with its specified pointing in the spacecraft system…”
Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission (2018, methodology): “ENAs strike a 15° inclined diamond-like carbon CS on a Si wafer converting ENAs into negative ions (Wurz et al. 1997, 2006; Scheer et al. 2005, 2006; Wieser et al. 2007; Fuselier et al. 2009b; Bzowski et al. 2012; Möbius et al. 2009; Bochsler et al. 2012; Park et al. 2014; Funsten et al. 2009a).”
The Interstellar Boundary Explorer High Energy (IBEX-Hi) Neutral Atom Imager (2009, methodology): “…similar in functional design, these sensors are optimized to measure the tenuous ENA flux across two overlapping energy ranges: the IBEX-Lo sensor (Fuselier et al. 2009, this issue) measures ENAs from ∼10 eV to 2 keV in eight energy steps, and the IBEX-Hi sensor measures ENAs from ∼380 eV to 6…”